Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU

The cubic-kilometer sized IceCube neutrino observatory is burieddeep in the glacial ice at the Earth’s South Pole. Its low-energyextension array DeepCore enables physicists to search indirectlyfor light Dark Matter (DM) particles with masses as low as tensof GeV/c2 situated within our home galaxy, t...

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Bibliographic Details
Main Author: Wolf, Martin
Format: Master Thesis
Language:English
Published: Stockholms universitet, Fysikum 2014
Subjects:
Online Access:http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104786
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spelling ftstockholmuniv:oai:DiVA.org:su-104786 2023-05-15T18:23:01+02:00 Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU Wolf, Martin 2014 application/pdf http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104786 eng eng Stockholms universitet, Fysikum Stockholm http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104786 info:eu-repo/semantics/openAccess Dark Matter Galactic Center IceCube DeepCore PINGU Astronomy Astrophysics and Cosmology Astronomi astrofysik och kosmologi Licentiate thesis, monograph info:eu-repo/semantics/masterThesis text 2014 ftstockholmuniv 2023-02-23T21:41:25Z The cubic-kilometer sized IceCube neutrino observatory is burieddeep in the glacial ice at the Earth’s South Pole. Its low-energyextension array DeepCore enables physicists to search indirectlyfor light Dark Matter (DM) particles with masses as low as tensof GeV/c2 situated within our home galaxy, the Milky Way. GeVneutrinos could be produced through DM particle annihilations,propagating to the Earth where they could be detected by IceCube. This licentiate thesis presents a search for Weakly Interacting Mas-sive Particles (WIMPs) with masses as low as 30 GeV/c2 in theGalactic center (GC) using the 79-string configuration of the IceCubeneutrino detector. Data from 319.7 live-days have been analyzedusing a cut-and-count analysis approach, and found to be consistentwith the background-only hypothesis with expected backgroundfrom atmospheric muons and neutrinos. Thus, upper limits wereset on the velocity averaged DM annihilation cross-section. The Precision IceCube Next Generation Upgrade (PINGU) as apossible future neutrino detector within DeepCore would reducethe neutrino energy detection threshold to a few GeV. In additionto the data analysis with DeepCore, a sensitivity study has beenconducted to investigate the performance of PINGU for indirectDM searches in the GC and the Sun. In the Sun WIMPs could begravitationally captured through elastic scattering off nucleons. Inthis thesis, we derive PINGU sensitivities for the velocity averagedDM annihilation cross-section of WIMPs in the GC, and for theSpin-Dependent (SD) and Spin-Independent (SI) WIMP-protonscattering cross-sections, under the assumption of thermodynamicequilibrium between the WIMP capturing and annihilation rate inthe Sun. IceCube Master Thesis South pole Stockholm University: Publications (DiVA) Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) Pingu ENVELOPE(-52.017,-52.017,67.067,67.067) South Pole
institution Open Polar
collection Stockholm University: Publications (DiVA)
op_collection_id ftstockholmuniv
language English
topic Dark Matter
Galactic Center
IceCube
DeepCore
PINGU
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
spellingShingle Dark Matter
Galactic Center
IceCube
DeepCore
PINGU
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
Wolf, Martin
Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
topic_facet Dark Matter
Galactic Center
IceCube
DeepCore
PINGU
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
description The cubic-kilometer sized IceCube neutrino observatory is burieddeep in the glacial ice at the Earth’s South Pole. Its low-energyextension array DeepCore enables physicists to search indirectlyfor light Dark Matter (DM) particles with masses as low as tensof GeV/c2 situated within our home galaxy, the Milky Way. GeVneutrinos could be produced through DM particle annihilations,propagating to the Earth where they could be detected by IceCube. This licentiate thesis presents a search for Weakly Interacting Mas-sive Particles (WIMPs) with masses as low as 30 GeV/c2 in theGalactic center (GC) using the 79-string configuration of the IceCubeneutrino detector. Data from 319.7 live-days have been analyzedusing a cut-and-count analysis approach, and found to be consistentwith the background-only hypothesis with expected backgroundfrom atmospheric muons and neutrinos. Thus, upper limits wereset on the velocity averaged DM annihilation cross-section. The Precision IceCube Next Generation Upgrade (PINGU) as apossible future neutrino detector within DeepCore would reducethe neutrino energy detection threshold to a few GeV. In additionto the data analysis with DeepCore, a sensitivity study has beenconducted to investigate the performance of PINGU for indirectDM searches in the GC and the Sun. In the Sun WIMPs could begravitationally captured through elastic scattering off nucleons. Inthis thesis, we derive PINGU sensitivities for the velocity averagedDM annihilation cross-section of WIMPs in the GC, and for theSpin-Dependent (SD) and Spin-Independent (SI) WIMP-protonscattering cross-sections, under the assumption of thermodynamicequilibrium between the WIMP capturing and annihilation rate inthe Sun. IceCube
format Master Thesis
author Wolf, Martin
author_facet Wolf, Martin
author_sort Wolf, Martin
title Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
title_short Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
title_full Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
title_fullStr Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
title_full_unstemmed Indirect Searches for Galactic Dark Matter with IceCube-DeepCore and PINGU
title_sort indirect searches for galactic dark matter with icecube-deepcore and pingu
publisher Stockholms universitet, Fysikum
publishDate 2014
url http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104786
long_lat ENVELOPE(-68.705,-68.705,-71.251,-71.251)
ENVELOPE(-52.017,-52.017,67.067,67.067)
geographic Milky Way
Pingu
South Pole
geographic_facet Milky Way
Pingu
South Pole
genre South pole
genre_facet South pole
op_relation http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104786
op_rights info:eu-repo/semantics/openAccess
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